An examination was made of earth based observations of optical color differences, infrared eclipse temperatures, and radar backscatter for Mare Serenitatis. Information is also included on orbital observations, physical properties of surface types, and correlation of surface types with geologic units. Differences in these remote observations are attributed to variations in chemical and minerological compositions.
Remote sensing of Mare Serenitatis
1973-01-01
Miscellaneous
No indication
English
The geology of the Mare Serenitatis region of the moon
NTRS | 1966
|Geology and deposits of the Serenitatis basin
NTRS | 1993
|Stratigraphy and Tectonics of Southeastern Serenitatis
NTRS | 1976
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